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Effect of Optical Depth on Study of Chemical Properties of Massive Star Forming Clumpsy
Zhou Jianjun; Li Runxia; Quan Donghui; Esimbek Jarken; He Yuxin; Li Dalei; Tang Xindi; Wu Gang; Ji Weiguang; Chang Zhengxue; Zhang Xia
2020
Source PublicationChinese Journal of Chemical Physics
ISSN1674-0068
Volume33Issue:1Pages:114-118
AbstractHere we present the study on chemical properties of massive star forming clumps using N_2H~+(1-0), H~(13)CO~+(1-0), HCN(1-0) and HN~(13)C(1-0) data from the literature Astron. Astrophys. 563, A97(2014). We found that abundances of H~(13)CO~+ and HN~(13)C are affected by H_2 column densities. As the median values of these two abundances increase by nearly 10 times from stages A to B, H~(13)CO~+ and HN~(13)C are suitable for tracing the evolution of massive star forming clumps. The order of rapidity in growth of abundances of all the four studied molecules from stages A to B, is H~(13)CO~+, HCN, HN~(13)C, and N_2H~+, from the highest to the lowest. Our results suggest that the observing optically thin molecular lines with high angular resolution are necessary to study the chemical evolution of massive star forming clumps.
Keyword恒星形成 团块 分子射电谱线 Stars formation Clumps Molecules Radio lines
Indexed ByCSCD
Language英语
CSCD IDCSCD:6671914
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Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/6523
Collection中国科学院新疆天文台
Affiliation中国科学院新疆天文台
First Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Zhou Jianjun,Li Runxia,Quan Donghui,et al. Effect of Optical Depth on Study of Chemical Properties of Massive Star Forming Clumpsy[J]. Chinese Journal of Chemical Physics,2020,33(1):114-118.
APA Zhou Jianjun.,Li Runxia.,Quan Donghui.,Esimbek Jarken.,He Yuxin.,...&Zhang Xia.(2020).Effect of Optical Depth on Study of Chemical Properties of Massive Star Forming Clumpsy.Chinese Journal of Chemical Physics,33(1),114-118.
MLA Zhou Jianjun,et al."Effect of Optical Depth on Study of Chemical Properties of Massive Star Forming Clumpsy".Chinese Journal of Chemical Physics 33.1(2020):114-118.
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